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| JOURNAL HOME | HELP | CONTACT PUBLISHER | SUBSCRIBE | ARCHIVE | SEARCH | TABLE OF CONTENTS |
1 U.S. Geological Survey, MS 989, 345 Middlefield Road, Menlo Park, California 94025, USA
| ABSTRACT |
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Geophysical modeling indicates that the source of the geophysical anomaly must extend to mid-crustal depths, perhaps reflecting a transition from Paleozoic crust in the southwest to Precambrian crust in the northeast, the presence of felsic intrusive rocks in the middle crust, or the edge of mid- to sub-crustal mafic intrusions related to late Tertiary magmatic underplating associated with hotspot magmatism.
These cases offer very different possibilities for the age, depth, and origin of the source of the geophysical anomaly, and they present distinct implications for crustal evolution in the northern Great Basin. For example, if the anomaly is due to a pre-Cenozoic basement structure, then its coincidence with the mid-Miocene northern Nevada rift suggests that the trend of the rift was guided by the pre-existing crustal structure. On the other hand, if the anomaly is related to Tertiary mafic intrusions, then the western limit of this magmatism may have been influenced by hotspot fracturing of the crust.
Keywords: gravity and magnetic anomalies northern Nevada rift epithermal gold deposits Battle Mountain–Eureka mineral trend Basin and Range Nevada
| INTRODUCTION |
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Geophysical studies in northern Nevada have resulted in several models for the origin and significance of a series of prominent geophysical features known as the northern Nevada rifts (NNRe, NNRc, NNRw, Fig. 1) (Glen and Ponce, 2002; Ponce and Glen, 2002). The originally named northern Nevada rift (Zoback and Thompson, 1978; Zoback et al., 1994), expressed by a prominent aeromagnetic anomaly herein referred to as the eastern northern Nevada rift (Figs. 1 and 2), extends from at least the Nevada-Oregon border to southeast Nevada (Blakely, 1988; Blakely and Jachens, 1991). Moreover, recent studies along the eastern northern Nevada rift and associated features to the west (Fig. 1) (John et al., 2000; Glen and Ponce, 2002; Ponce and Glen, 2002) have indicated that the northern Nevada rift is a much wider feature than previously thought. These studies expand on its relationship to known and potential mineral resources along its trend, and they indicate that the feature extends northward well beyond the Nevada-Oregon border.
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| PREVIOUS WORK |
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5 km) aeromagnetic data, Blakely and Jachens (1991) suggested that the northern Nevada rift extends much farther to the south and that the rift also follows a well-defined isostatic and basement gravity gradient. Zoback et al. (1994) reassessed the northern Nevada rift in light of more recent data and reaffirmed their earlier interpretations of the northern Nevada rift as an indicator of the mid-Miocene stress direction. A study by John et al. (2000) have shown that the northern Nevada rift is prominently expressed in gravity, magnetic, and other derivative geophysical maps, that it is an arcuate and a much wider feature than previously thought, and that it correlates to known epithermal deposits. The eastern northern Nevada rift and related parallel magnetic anomalies to the west (NNRc, NNRw, Fig. 2) are associated with epithermal gold deposits in northern Nevada, extend well beyond the Nevada-Oregon border, and converge at a point along the Oregon-Idaho border at latitude 44°, which is interpreted to be the inception site of the Yellowstone hotspot (see Glen and Ponce, 2002; Ponce and Glen, 2002). Grauch et al. (1995) were the first to suggest that the Battle Mountain–Eureka mineral trend, an alignment of a wide range of gold deposits including sediment-hosted and pluton-related gold deposits (Roberts, 1966), corresponds to a basement gravity gradient and that this boundary could be of Jurassic age or older because of an associated alignment of Jurassic plutons and possible folds. Grauch et al. (2003a, 2003b) presented additional evidence that the Battle Mountain–Eureka mineral trend correlates to a major crustal-scale fault zone primarily based on magnetotelluric and radiogenic isotope data (also see Tosdal et al., 2000; Crafford and Grauch, 2002; Rodriguez et al., 2007). Both the Battle Mountain–Eureka mineral trend and the northern Nevada rift occur in a transition zone between the craton to the east and oceanic crust to the west, where the intervening continental margin is defined by the initial 87Sr/86Sr = 0.7060 isopleth (e.g., Tosdal et al., 2000) (Fig. 1). Ponce and Glen (2002) showed that the western edge of the northern Nevada rift also occurs along a large-scale crustal feature, part of which is coincident with the central part of the Battle Mountain–Eureka mineral trend (Figs. 2 and 3).
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| GEOPHYSICAL DATA AND METHODOLOGY |
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An isostatic gravity map of the region (Fig. 3) was derived from a statewide gravity data compilation of Nevada (Ponce, 1997) and augmented with over 2000 new gravity stations collected throughout northern Nevada (e.g., Jewel et al., 2000; Sanger and Ponce, 2003; Scheirer, 2005; Tilden et al., 2005, 2006; Mankinen et al., 2006). All gravity data were reduced using standard gravity methods (e.g., Dobrin and Savit, 1988; Blakely, 1995) to yield isostatic gravity anomalies that emphasize features in the middle to upper crust, having removed long-wavelength variations in the gravity field related to topography (e.g., Jachens and Roberts, 1981; Simpson et al., 1986).
Gravity Inversion and Basement Gravity
The isostatic gravity map of northern Nevada (Fig. 3) is dominated by anomalies related to low-density basin-filling materials. It is therefore desirable to remove these effects to highlight gravity anomalies associated with pre-Cenozoic basement rocks. This was achieved by using an iterative gravity inversion technique originally developed by Jachens and Moring (1990) and discussed in more detail by them and others (e.g., Blakely and Jachens, 1991; Saltus and Jachens, 1995; Jachens et al., 1996). The inversion process essentially separates the isostatic gravity field into two components: the gravity field generated by less-dense overlying Cenozoic deposits and the gravity field generated by intrusions and pre-Cenozoic basement rocks. The resulting basin gravity field can be used to determine the thickness of Cenozoic deposits in the study area (Fig. 4), and the basement gravity field can be used to identify geophysical features within the basement rocks (Fig. 5). The gravity inversion was constrained by simplified geologic data (Stewart and Carlson, 1978), a density-depth function for Cenozoic deposits (e.g., Jachens and Moring, 1990; Saltus and Jachens, 1995; Jachens et al., 1996); drill-hole information (e.g., Ponce and Moring, 1998; Hess, 2004), and other geophysical constraints (e.g., magnetotelluric data; Rodriguez and Williams, 2002).
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| GEOPHYSICAL EXPRESSION |
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1000 km. The source of the magnetic anomaly is essentially vertical, and the longer wavelengths (Fig. 6A)
12–15 km wide in north-central Nevada. Alongside and parallel to the anomaly, magnetic data (Fig. 2) indicate additional magnetic sources associated with the northern Nevada rift. This is particularly evident along the east side of the northern Shoshone Range, as revealed by two- and three-dimensional modeling (Watt et al., 2007). These modeling studies indicate that the eastern northern Nevada rift reflects a major crustal feature that extends to at least mid-crustal depths, and, combined with geologic data, they indicate that the northern Nevada rift and vicinity is characterized by complex structures that could play an important role in localizing fluid flow and mineralization.
The central part of the eastern northern Nevada rift is also characterized by a series of left-stepping segmented magnetic anomalies (Fig. 2A). These segments may reflect later, perhaps Late Miocene, offsets along NE-striking left-lateral cross faults (e.g., Mabey, 1966; Zoback et al., 1994; John et al., 2000). Lateral offsets along four main cross faults range from 1.6 to 3.4 km (Zoback et al., 1994). These segments, of which there may be six or more (Figs. 2A and 2B), vary in length from
11 to 41 km, and average
27 km. The largest intervening gaps or distances along strike between these segments occur in Boulder Valley, with a length of
4 km, and in Crescent Valley, with a length of
7 km (BV and CV, black and white lines in Fig. 2B).
Although a prominent aeromagnetic anomaly delineates (and defines) the northern Nevada rift, the rift is also expressed in gravity and other derivative gravity maps (e.g., Eaton et al., 1978; Mabey et al., 1983; Blakely, 1988; Saltus, 1988; Blakely and Jachens, 1991; Grauch et al., 1995; Ponce and Glen, 2002). An improved isostatic gravity map (Fig. 3), which includes
2000 recently collected gravity stations in northern Nevada, highlights the steep gravity gradient in central Nevada that is coincident with the western margin of the northern Nevada rift.
| ASSOCIATED MINERAL DEPOSITS |
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The prominent crustal feature along the northern Nevada rift (R-CF, Fig. 1) is also adjacent to the Battle Mountain–Eureka mineral trend, a Late Cretaceous to Tertiary mineral trend that contains a wide range of mineral deposits, including sediment-hosted as well as pluton-related gold deposits (Roberts, 1966). The Battle Mountain–Eureka mineral trend includes deposits in Buffalo Valley, Battle Mountain, Cortez-Pipeline, Eureka, and White Pine mining districts (e.g., Wallace et al., 2004a). Deposits along the Battle Mountain–Eureka mineral trend were used to define a least-squares regression line (yellow line, Fig. 1) as well as a rectangular area depicting their horizontal extent (transparent rectangle, Fig. 1). Not surprisingly, the horizontal extent of the Battle Mountain–Eureka mineral trend thus defined is very similar to that originally shown by Roberts (1966) from Battle Mountain to southeast of Eureka, Nevada (dashed line, Fig. 1). The rift crustal feature is especially coincident with the central part of the Battle Mountain–Eureka mineral trend, in between but exclusive of Battle Mountain and Eureka. South of Eureka, the rift crustal feature diverges from the Battle Mountain–Eureka mineral trend, based on mineral deposit locations considered part of the trend (e.g., Wallace et al., 2004a). An associated belt of high arsenic values along the Battle Mountain–Eureka mineral trend, which probably reflects the mobilization of arsenic by hydrothermal fluids from associated plutons, faulting, and mineral deposits (Ludington et al., 2006), also indicates that the Battle Mountain–Eureka mineral trend and the rift crustal feature are separate features south of Eureka. Interestingly, the northern Nevada rift itself is not associated with an arsenic anomaly, even though it is associated with arsenic-rich epithermal gold deposits and reflects a zone of crustal rifting (Ludington et al., 2006).
| DISCUSSION |
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The rift crustal feature appears to be subparallel to and partially coincident with the inferred Battle Mountain–Eureka crustal fault zone (Grauch et al., 1995, 2003a). This is particularly evident along the central part of the Battle Mountain–Eureka mineral trend, southeast of Battle Mountain and northwest of Eureka, Nevada. The association of the northern Nevada rift and the central part of the Battle Mountain–Eureka crustal fault zone suggests that the northern Nevada rift, at least in part, preferentially followed a pre-existing structure. If so, this could bring into question whether or not the northern Nevada rift reflects the mid-Miocene direction of least principal stress (Zoback and Thompson, 1978; Zoback et al., 1994; Glen and Ponce, 2002). On the other hand, the curvilinear pattern of the eastern northern Nevada rift and the parallel features to the west (NNRw, NNRc, Figs. 1 and 2), combined with the results of a superimposed simple model of hotspot and regional stress fields (Glen and Ponce, 2002), which yield a radiating stress pattern near the hotspot that spirals into the regional stress field at distance, indicate that the northern Nevada rift likely reflects the mid-Miocene least principal stress direction in north-central Nevada, as first suggested by Zoback (1978), and that it only exploited the Battle Mountain–Eureka crustal fault zone where the two are coincident. During mid-Miocene time, the least principal stress direction was N65°–70°E, essentially perpendicular to the trend of the eastern northern Nevada rift (N22°W) in north-central Nevada, and between ca. 10 and 6 Ma, the least principal stress direction changed to about N60°–70°W, consistent with younger NNE-striking fault offsets along the northern Nevada rift (e.g., Zoback, 1978; Zoback et al., 1994).
The rift crustal feature and the Battle Mountain–Eureka mineral trend clearly deviate from one another only at Battle Mountain and southeast of and including Eureka. Near Battle Mountain, the Battle Mountain–Eureka mineral trend is offset by
15 km and skewed by
15–20°W (counterclockwise) from the N22°W trend of the northern Nevada rift. However, if the rift crustal feature and the central part of the Battle Mountain–Eureka crustal fault zone are in fact the same feature, increasing left-lateral offsets on range-bounding cross faults along the rift combined with the opening of Reese River Valley, a prominent depocenter more than 2 km thick (Fig. 5) that occurs between the northern Nevada rift and the Battle Mountain–Eureka mineral trend, could help to explain the divergence of the deposits at Battle Mountain from the rift crustal feature. This is supported by large-scale extension to the west (Wallace, 1991) and southwest (Colgan et al., 2008) of the northern Nevada rift in this area. The magnetic anomaly along the northern Nevada rift appears to be segmented (Fig. 2), and left-lateral offsets (up to several kilometers) by northeast-striking cross faults are exhibited (e.g., Mabey, 1966; Muffler, 1964; Mabey et al., 1978; Zoback, 1978; Zoback et al., 1994). Zoback (1978) estimated that extension may be up to 12 km (or
20%) in the vicinity of the northern Nevada rift. In addition, the Reese River Valley is one of several basins in central Nevada obviously influenced by the rift crustal feature (Fig. 4), as first noted by Blakely and Jachens (1991), suggesting that the northern Nevada rift affected basin development. If so, the northern Nevada rift likely impacts water resources as well as mineral resources in north-central Nevada.
Alternatively, the left-stepping segmented pattern of magnetic anomalies along the eastern northern Nevada rift (black and white lines, Fig. 2), which is particularly noticeable between the Sheep Creek Range and Eureka, may reflect primary en echelon emplacement of the northern Nevada rift—i.e., originating at the time of intrusion. The left-stepping mid-Miocene Sawtooth dike (black rectangle, Fig. 2), which is within the magnetic anomaly associated with the northern Nevada rift, is suggestive of this, since it is considered to be the result of transform rather than left-lateral fault motion (Zoback and Thompson, 1978; Zoback et al., 1979). If so, this would imply that the northern Nevada rift and its associated mafic intrusions have been virtually unaffected by Basin and Range extension. Conversely, Livaccari (in Zoback et al., 1979) and Wallace (2000) have pointed out that this offset of the Sawtooth dike may be related to minor left-lateral movements along an ENE-striking fault, where the ends of the dike are faulted and dragged after emplacement, and where a small piece of the dike in the fault zone exhibits counterclockwise rotation consistent with left-lateral motion. In any case, the northern Nevada rift and associated basement structure probably act like a rigid keel in the crust, prohibiting extension across it and influencing subsequent Basin and Range development. Colgan et al. (2008) indicate that the basement gravity high in north-central Nevada, northeast of the northern Nevada rift (Fig. 5), partly correlates to an unextended mid-Miocene terrane that has acted as a rigid block and resisted extension. The faulting that possibly controlled the present location of the Battle Mountain deposits would then be necessarily restricted westward of the northern Nevada rift in a highly extended area.
At Eureka, deposits along the Battle Mountain–Eureka mineral trend are clearly on the east side of the rift crustal feature south of about latitude 39.5°N, a location that also marks a dramatic change in the character of the associated magnetic and basement gravity anomalies (Figs. 2 and 5) (e.g., Blakely, 1988; Blakely and Jachens, 1991; Zoback et al., 1994). Here, deposits along the Battle Mountain–Eureka mineral trend may, in part, be a local phenomena related to the intersection of the NW-trending rift crustal feature and a NE-trending basement gravity feature (V-shaped anomaly, Fig. 6C
). Interestingly, there is a difference in the ages of pluton-related deposits along the Battle Mountain–Eureka mineral trend: deposits at Eureka are predominantly Cretaceous, whereas those near Battle Mountain are predominantly Eocene (e.g., Table 7-1, in Theodore et al., 2004). Ages of Carlin-type (sediment-hosted) deposits associated with the Battle Mountain–Eureka mineral trend are difficult to determine but, in general are similar in age and range from 42 to 30 Ma for the Great Basin (Hofstra et al., 1999; Arehart et al., 2003). For example, Yigit et al. (2003) indicated that mineralization at the Gold Bar deposit along the Battle Mountain–Eureka mineral trend in the Roberts Mountains (Fig. 1), is between 37.5 and 24 Ma. Deposits farther southeast of Eureka are not strongly associated with a prominent geophysical feature and may be unrelated to the rift crustal feature, Battle Mountain–Eureka mineral trend, or Battle Mountain–Eureka crustal fault zone.
Although the broad basement gravity feature that extends across northern Nevada (V-shaped anomaly, Figs. 5 and 6C
) may be related to a pre-Cenozoic geologic structure (e.g., Grauch et al., 1995, 2003a; Tosdal et al., 2000), it is also continuous with the gravity expression of the Snake River Plain apron of volcanic rocks (Glen et al., 2004) and with the NE extension of the Battle Mountain heat-flow high (e.g., Lachenbruch and Sass, 1978; Sass et al., 1981; Blakely, 1988), which suggest that the source of the basement gravity anomaly is hotspot-related, mid- to subcrustal mafic intrusions and underplating. Either way, the basement crustal boundary probably played a major role in controlling and influencing subsequent mineralization and tectonic events in north-central Nevada (e.g., Grauch et al., 1995, 2003a; Hildenbrand et al., 2000; Tosdal et al., 2000; Crafford and Grauch, 2002).
| CONCLUSIONS |
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At Battle Mountain and southeast of and including Eureka, the geophysical feature and the Battle Mountain–Eureka mineral trend clearly deviate from one another. If the crustal faults along the mid-Miocene northern Nevada rift and the central part of the Eocene and older Battle Mountain–Eureka mineral trend are in fact the same feature, deposits at a greater distance from the crustal feature associated with the northern Nevada rift at Battle Mountain could be explained by postemplacement tectonic events. However, those deposits near Eureka may be related to the intersection of two crustal-scale faults. The association of the northern Nevada rift and the central part of the crustal fault zone along the Battle Mountain–Eureka mineral trend suggests that the location of the northern Nevada rift was at least in part preferentially influenced by a pre-existing structure.
Although the broad basement gravity feature in northern Nevada is likely related to a pre-Cenozoic geologic structure, its continuity with a broad gravity high extending from the Snake River Plain suggests that the source of the anomaly is, in part, related to hotspot magmatism. This implies that the extent of under-plating was either limited by northern Nevada rift diking that tapped subcrustal magmas or that hotspot magmatism was guided and influenced by pre-existing structures. In any case, these large-scale crustal features are important to understanding the metallogeny, tectonics, and magmatism of the Great Basin, as well as water and environmental issues.
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| ACKNOWLEDGMENTS |
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| Footnotes |
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MANUSCRIPT RECEIVED BY THE SOCIETY 30 March 2007
REVISED MANUSCRIPT RECEIVED 28 September 2007
MANUSCRIPT ACCEPTED 2 October 2007
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